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Mostly Mute Monday: NASA’s Greatest Observatories View The Galactic Center

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With Hubble, Spitzer and Chandra combined, we get a view like no other.

“But I see it differently now. There has to be a middle. Without it, nothing can truly be whole. Because it is not just the space between, but also what holds everything together.” –Sarah Dessen

Image credit: NASA, ESA, and Q.D. Wang (University of Massachusetts, Amherst), via http://hubblesite.org/newscenter/archive/releases/2009/02/image/b/.
Image credit: NASA, ESA, and Q.D. Wang (University of Massachusetts, Amherst), via http://hubblesite.org/newscenter/archive/releases/2009/02/image/b/.
Image composite credit: NASA, Jet Propulsion Laboratory, and S. Stolovy (Spitzer Science Center/Caltech); NASA, ESA, Q.D. Wang (University of Massachusetts, Amherst), and S. Stolovy (Caltech), via http://hubblesite.org/newscenter/archive/releases/2009/02/image/d/.
Image composite credit: NASA, Jet Propulsion Laboratory, and S. Stolovy (Spitzer Science Center/Caltech); NASA, ESA, Q.D. Wang (University of Massachusetts, Amherst), and S. Stolovy (Caltech), via http://hubblesite.org/newscenter/archive/releases/2009/02/image/d/.
Image credit: NASA/UMass/D.Wang et al.; Chandra X-Ray Observatory / Smithsonian Astrophysical Observatory.
Image credit: NASA/UMass/D.Wang et al.; Chandra X-Ray Observatory / Smithsonian Astrophysical Observatory.
Image credit: NASA/JPL-Caltech/ESA/CXC/STScI, via http://photojournal.jpl.nasa.gov/catalog/PIA12348.
Image credit: NASA/JPL-Caltech/ESA/CXC/STScI, via http://photojournal.jpl.nasa.gov/catalog/PIA12348.

Although the galactic center is practically invisible in visible light due to the copious amounts of light-blocking dust, the dust grains that are present are of insufficient size to block both much shorter (X-ray) and much longer-wavelength (infrared) light. Thanks to a combination of Hubble’s near-infrared (NICMOS) instrument, the Spitzer Space Telescope (mid-and-far IR) and the Chandra X-ray observatory, a multiwavelength panoramic view of the region surrounding the galactic center has been constructed.

What we find inside is a tumultuous region of dense stars, the gas blown off from recent stellar deaths, the neutral atoms that will collapse to form new stars, and a myriad of intense, high-energy sources that correspond to neutron stars and black holes. Perhaps most spectacularly, there’s a four million solar mass black hole at our galaxy’s center, illuminated uniquely (below) by each of the three great observatories. By combining the data from all of them, we get a unique look at the astrophysical signatures emitted by the closest supermassive black hole to us in the Universe.

Image credit: NASA, ESA, and Q.D. Wang (University of Massachusetts, Amherst), via http://hubblesite.org/newscenter/archive/releases/2009/02/image/b/.
Image composite credit: NASA, Jet Propulsion Laboratory, and S. Stolovy (Spitzer Science Center/Caltech); NASA, ESA, Q.D. Wang (University of Massachusetts, Amherst), and S. Stolovy (Caltech), via http://hubblesite.org/newscenter/archive/releases/2009/02/image/d/.
Image credit: NASA/UMass/D.Wang et al.; Chandra X-Ray Observatory / Smithsonian Astrophysical Observatory.
Image credit: NASA/JPL-Caltech/ESA/CXC/STScI, via http://photojournal.jpl.nasa.gov/catalog/PIA12348.

Mostly Mute Monday tells the story of a single phenomenon in images, videos, and 200 words, maximum. To celebrate Hubble’s 25th anniversary, the month of April, 2015, will focus exclusively on objects imaged with the Hubble Space Telescope.

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